For different \(\rho _0\) , \(\rho _q\)  and \(j\) , the numerical values for
the observables are listed in Table 1. One can see that our results
reduce to those in the four-dimensional Schwarzschild black hole as
\(\rho _0\longrightarrow 0\) . Also our results are in agreement with the
results of Ref. [1]} in the limit \(\rho _q\longrightarrow 0\) 
and in the limit \(j\longrightarrow 0\) , the results of Ref.
[2]} are recovered.
